ABSTRACT
Solar quiet current (𝑆𝑞) and Equatorial Electrojet (EEJ) are
two current systems which are produced
by electric current in the ionosphere.
The enhancement of the horizontal magnetic field is the EEJ.
This research is needed for monitoring
equatorial geomagnetic current which causes atmospheric
instabilities and affects high
frequency and satellite communication. This study presents the
longitudinal and latitudinal variation
of equatorial electrojet signature at stations within the
96°𝑚𝑚 𝑎𝑛𝑑 210°𝑚𝑚 African and Asian sectors
respectively during quiet condition. Data from
eleven observatories were used for
this study. The aim of this study is to investigate the equatorial
variation of the solar quite (𝑆𝑞) current, as well as determine the
longitudinal and latitudinal
magnetic signatures on the EEJ at some
African and Asian sectors under quiet condition. The
objectives of the study therefore are
to: Determine the longitudinal and latitudinal geomagnetic field
variations during solar quiet
conditions along the 96° 𝑎𝑛𝑑 210°𝑚𝑚; Investigate monthly variation
and diurnal transient seasonal
variation; Measure the strength of the EEJ at stations within the same
longitudinal sectors of 96° 𝑎𝑛𝑑 210° 𝑚𝑎𝑔𝑛𝑒𝑡𝑖𝑐 𝑚𝑒𝑟𝑖𝑑𝑖𝑎𝑛; and find out the factors responsible
for
the longitudinal and latitudinal
variation of EEJ under solar quiet condition. Horizontal (𝐻)
component of geomagnetic field for the
year 2008 from Magnetic Data Acquisition System
(MAGDAS) network were used for the
study. The International Quiet Days (IQDs) were used to
identify quiet days. Daily baseline
values for each of the geomagnetic element 𝐻, can be obtained
from 𝐻0 = 1
⁄2 (𝐻24 + 𝐻1) where 𝐻0 is the dailybaseline. The daily
baseline was subtracted from
the hourly values to get the hourly
departure from midnight for a particular day𝑑𝐻 = 𝐻𝑡 − 𝐻0 where
𝑡 = 1 𝑡𝑜 24 𝑎𝑛𝑑 𝑑𝐻 gives the measure of the hourly
amplitude of the variation of 𝐻. The monthly
average of the diurnal variation was
found. The seasonal variation of 𝑑𝐻 was found by averaging the
monthly means for Lloyd’s season.
Results showed that: The longitudinal and latitudinal variation in
the 𝑑𝐻 differs in magnitude from one station
to another within the same longitude due to the
difference in the influence of the EEJ
on them, which depends on how far from or near (latitudinal
difference) they are to the EEJ band
(confined within ±3° 𝑙𝑎𝑡𝑖𝑡𝑢𝑑𝑒) wherein the EEJ current flows
eastwards; The highest monthly
longitudinal variation of EEJ is 92 𝑛𝑇 at DAV and TIR during
September equinox. This high amplitude
at DAV and TIR compared with the other 9 stations, showed
the presence of higher electric
current (equatorial electrojet) in the ionosphere flowing over DAV and
TIR. Thus the high magnitude could possibly be due to a
greater width of the electrojet over the
stations. The variation pattern for
daily, monthly and seasonal variation were found to be similar;
The magnitude of EEJ strength at
stations within the same specified longitude differ where the EEJ
strength at ILR is maximum with
𝑑𝐻
of 55 𝑛𝑇
at about 1100 LT and maximum EEJ strength at DAV
is 93 𝑛𝑇 at about 1200LT which is the
highest for the specified year; The possible factors responsible
for the variation of EEJ is seen to be
the ionospheric processes and physical structure such as wind
and conductivity. The 𝑑𝐻 value peaks between 1000 LT and
0200 LT for all the plots and varies with
longitude and with latitude. The EEJ
value for equinoctial months is seen to be higher than those of
solstice months where the buildup
flank is steeper in the morning hours than in the evening hours.
TOPIC: THE STUDY OF LONGITUDINAL AND LATITUDINAL VARIATION OF EQUATORIAL ELECTROJET SIGNATURE AT STATIONS WITHIN THE 96°MM AND 210°MM AFRICAN AND ASIAN SECTORS RESPECTIVELY UNDER QUIET CONDITION
Chapters: 1 - 5
Delivery: Email
Delivery: Email
Number of Pages: 68
Price: 3000 NGN
In Stock

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